MOJAVE Sample: 0133+388

Common Name:	B3 0133+388	MOJAVE 15 GHz \|	VLBA 1.4 GHz:
B1950 Name:	0133+388
J2000 Name:	J0136+3905
R.A. and Dec. (J2000):	1h36m32.598s +39d5'59.199"
AGN Class:	HSP BL Lac
Redshift:	Unknown
Luminosity Distance:	Unknown
Radio Spectrum:	Flat
Gamma-ray Association	LAT: Y, EGRET: N, TeV: Y
Kpc-scale morphology:	Unknown
Jet Speed:	Maximum: 40 ± 46 μas/y ; Median: N/A ; Piner and Edwards 2018
Separation Versus Time Plot:	Not available
Stacked 15 GHz Stokes I VLBA images: Natural weight: Not Available Circular Beam: Not Available Tapered Beam: Not Available Stacked 15 GHz Polarization VLBA images: Rotation Measure 8-15 GHz Map: \| Not available \| Spectral Index 8-15 GHz Map: \| Not available \|	VLBA 23 GHz:	Kpc-scale:

Fermi LAT and 15 GHz VLBA Light Curves	VLBA 43 GHz:	Multiepoch Radio Spectrum:

Comments:	LAT_1FM weak sample; Nillson et al. 2012 get z > 0.4, Paiano 2017 get z > 0.27

Common Name:

B3 0133+388

MOJAVE 15 GHz |

VLBA 1.4 GHz:

R.A. and Dec. (J2000):

1h36m32.598s
+39d5'59.199"

HSP BL Lac

Unknown

Unknown

Flat

Gamma-ray Association

LAT: Y, EGRET: N, TeV: Y

Kpc-scale morphology:

Unknown

Jet Speed:

Maximum: 40 ± 46 μas/y ;
Median: N/A ;
Piner and Edwards 2018

Separation Versus Time Plot:

Not available

Stacked 15 GHz Stokes I VLBA images:
Natural weight: Not Available
Circular Beam: Not Available
Tapered Beam: Not Available

Stacked 15 GHz Polarization VLBA images:

Rotation Measure 8-15 GHz Map: | Not available |

Spectral Index 8-15 GHz Map: | Not available |

VLBA 23 GHz:

Kpc-scale:

Fermi LAT and 15 GHz VLBA Light Curves

VLBA 43 GHz:

Multiepoch Radio Spectrum:

Comments:

LAT_1FM weak sample; Nillson et al. 2012 get z > 0.4, Paiano 2017 get z > 0.27

If you use these data in a publication, we ask that you please contact us so we can add a link to the list of external MOJAVE publications, and ask that you cite Lister et al., 2018, ApJS, 234, 12 and include the following acknowledgment: "This research has made use of data from the MOJAVE database that is maintained by the MOJAVE team (Lister et al. 2018)"

Important Note: The MOJAVE team, working with the OVRO 40m AGN monitoring team checks and adjusts the flux density scaling of the MOJAVE VLBA data for possible systematics based on near-simultaneous OVRO 40m measurements at 15 GHz. Asterisked entries below denote epochs that have not yet been checked and corrected.

Epoch (YYYY-MM-DD)	VLBA Code	VLBA I (mJy)	VLBA P (mJy)	VLBA P (%)	VLBA EVPA (deg.)	I Image (Nat. Weight)	Visibility Data	Stokes I Radplot	Polarization Image	Full Montage
2010-11-29	BL149CY	7	< 2.6	< 347.6		FITS PNG PDF	UVF	PNG PDF	p:PNG p:PDF f:PNG f:PDF	PNG